Recherche
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How Measurements of Rate Coefficients at Low Temperature Increase the Predictivity of Photochemical Models of Titan's Atmosphere
(Journal of Physical Chemistry A. vol. 113, n° 42, pp. 11227-11237, 2009)Article de revue -
Photochemistry of C3Hp hydrocarbons in Titan's stratosphere revisited
(Astronomy and Astrophysics - A&A. vol. 552, pp. 132, 2013-04)Article de revue -
The photochemical production of aromatics in the atmosphere of Titan
(Icarus. vol. 329, pp. 55-71, 2019)Article de revue -
High-temperature measurements of VUV-absorption cross sections of CO2 and their application to exoplanets
(Astronomy and Astrophysics - A&A. vol. 551, pp. id.A131, 2013)Article de revue -
A chemical model for the atmosphere of hot Jupiters
(Astronomy and Astrophysics - A&A. vol. 546, pp. id.A43, 19 pp, 2012)Article de revue -
The impact of atmospheric circulation on the chemistry of the hot Jupiter HD 209458b
(Astronomy and Astrophysics - A&A. vol. 548, pp. id.A73, 8 pp., 2012)Article de revue -
A cometary origin for CO in the stratosphere of Saturn?
(Astronomy and Astrophysics - A&A. vol. 510, n° A88, pp. -, 2010)Article de revue -
First observation of CO at 345 GHz in the atmosphere of Saturn with the JCMT. New constaints on its origin
(Icarus. vol. 203, n° 2, pp. 531-540, 2009)Article de revue -
CO in the atmospheres of Saturn. Observations at millimeter and submillimeter wavelengths.
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